Misaligned Rotations of the Envelope, Outflow, and Disks in the Multiple Protostellar System of VLA 1623–2417: FAUST. III

dc.citation.articleNumber54en_US
dc.citation.issueNumber1en_US
dc.citation.journalTitleThe Astrophysical Journalen_US
dc.citation.volumeNumber927en_US
dc.contributor.authorOhashi, Satoshien_US
dc.contributor.authorCodella, Claudioen_US
dc.contributor.authorSakai, Namien_US
dc.contributor.authorChandler, Claire J.en_US
dc.contributor.authorCeccarelli, Ceciliaen_US
dc.contributor.authorAlves, Felipeen_US
dc.contributor.authorFedele, Davideen_US
dc.contributor.authorHanawa, Tomoyukien_US
dc.contributor.authorDurán, Auroraen_US
dc.contributor.authorFavre, Cécileen_US
dc.contributor.authorLópez-Sepulcre, Anaen_US
dc.contributor.authorLoinard, Laurenten_US
dc.contributor.authorMercimek, Seymaen_US
dc.contributor.authorMurillo, Nadia M.en_US
dc.contributor.authorPodio, Lindaen_US
dc.contributor.authorZhang, Yichenen_US
dc.contributor.authorAikawa, Yurien_US
dc.contributor.authorBalucani, Nadiaen_US
dc.contributor.authorBianchi, Eleonoraen_US
dc.contributor.authorBouvier, Mathildeen_US
dc.contributor.authorBusquet, Gemmaen_US
dc.contributor.authorCaselli, Paolaen_US
dc.contributor.authorCaux, Emmanuelen_US
dc.contributor.authorCharnley, Stevenen_US
dc.contributor.authorChoudhury, Spandanen_US
dc.contributor.authorCuello, Nicolasen_US
dc.contributor.authorSimone, Marta Deen_US
dc.contributor.authorDulieu, Francoisen_US
dc.contributor.authorEvans, Lucyen_US
dc.contributor.authorFeng, Siyien_US
dc.contributor.authorFontani, Francescoen_US
dc.contributor.authorFrancis, Loganen_US
dc.contributor.authorHama, Tetsuyaen_US
dc.contributor.authorHerbst, Ericen_US
dc.contributor.authorHirano, Shingoen_US
dc.contributor.authorHirota, Tomoyaen_US
dc.contributor.authorImai, Muneakien_US
dc.contributor.authorIsella, Andreaen_US
dc.contributor.authorJímenez-Serra, Izaskunen_US
dc.contributor.authorJohnstone, Dougen_US
dc.contributor.authorKahane, Claudineen_US
dc.contributor.authorGal, Romane Leen_US
dc.contributor.authorLefloch, Bertranden_US
dc.contributor.authorMaud, Luke T.en_US
dc.contributor.authorMaureira, María Joséen_US
dc.contributor.authorMenard, Francoisen_US
dc.contributor.authorMiotello, Annaen_US
dc.contributor.authorMoellenbrock, Georgeen_US
dc.contributor.authorMori, Shojien_US
dc.contributor.authorNakatani, Riouheien_US
dc.contributor.authorNomura, Hidekoen_US
dc.contributor.authorOba, Yasuhiroen_US
dc.contributor.authorO'Donoghue, Rossen_US
dc.contributor.authorOkoda, Yukien_US
dc.contributor.authorOspina-Zamudio, Juanen_US
dc.contributor.authorOya, Yokoen_US
dc.contributor.authorPineda, Jaimeen_US
dc.contributor.authorRimola, Alberten_US
dc.contributor.authorSakai, Takeshien_US
dc.contributor.authorSegura-Cox, Dominiqueen_US
dc.contributor.authorShirley, Yancyen_US
dc.contributor.authorSvoboda, Brianen_US
dc.contributor.authorTaquet, Vianneyen_US
dc.contributor.authorTesti, Leonardoen_US
dc.contributor.authorVastel, Charlotteen_US
dc.contributor.authorViti, Serenaen_US
dc.contributor.authorWatanabe, Naokien_US
dc.contributor.authorWatanabe, Yoshimasaen_US
dc.contributor.authorWitzel, Arezuen_US
dc.contributor.authorXue, Cien_US
dc.contributor.authorZhao, Boen_US
dc.contributor.authorYamamoto, Satoshien_US
dc.date.accessioned2022-04-15T14:45:24Zen_US
dc.date.available2022-04-15T14:45:24Zen_US
dc.date.issued2022en_US
dc.description.abstractWe report a study of the low-mass Class 0 multiple system VLA 1623AB in the Ophiuchus star-forming region, using H13CO+ (J = 3–2), CS (J = 5–4), and CCH (N = 3–2) lines as part of the ALMA Large Program FAUST. The analysis of the velocity fields revealed the rotation motion in the envelope and the velocity gradients in the outflows (about 2000 au down to 50 au). We further investigated the rotation of the circumbinary VLA 1623A disk, as well as the VLA 1623B disk. We found that the minor axis of the circumbinary disk of VLA 1623A is misaligned by about 12° with respect to the large-scale outflow and the rotation axis of the envelope. In contrast, the minor axis of the circumbinary disk is parallel to the large-scale magnetic field according to previous dust polarization observations, suggesting that the misalignment may be caused by the different directions of the envelope rotation and the magnetic field. If the velocity gradient of the outflow is caused by rotation, the outflow has a constant angular momentum and the launching radius is estimated to be 5–16 au, although it cannot be ruled out that the velocity gradient is driven by entrainments of the two high-velocity outflows. Furthermore, we detected for the first time a velocity gradient associated with rotation toward the VLA 16293B disk. The velocity gradient is opposite to the one from the large-scale envelope, outflow, and circumbinary disk. The origin of its opposite gradient is also discussed.en_US
dc.identifier.citationOhashi, Satoshi, Codella, Claudio, Sakai, Nami, et al.. "Misaligned Rotations of the Envelope, Outflow, and Disks in the Multiple Protostellar System of VLA 1623–2417: FAUST. III." <i>The Astrophysical Journal,</i> 927, no. 1 (2022) IOP Publishing: https://doi.org/10.3847/1538-4357/ac4cae.en_US
dc.identifier.digitalOhashi_2022_ApJ_927_54en_US
dc.identifier.doihttps://doi.org/10.3847/1538-4357/ac4caeen_US
dc.identifier.urihttps://hdl.handle.net/1911/112077en_US
dc.language.isoengen_US
dc.publisherIOP Publishingen_US
dc.rightsOriginal content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleMisaligned Rotations of the Envelope, Outflow, and Disks in the Multiple Protostellar System of VLA 1623–2417: FAUST. IIIen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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